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Improved Value for the Gamow-Teller Strength of the Sn100 Beta Decay
dc.creator | Lubos, D | |
dc.creator | Park, J | |
dc.creator | Faestermann, T | |
dc.creator | Gernhäuser, R | |
dc.creator | Baba, H | |
dc.creator | Blank, B | |
dc.creator | Blazhev, A | |
dc.creator | Boutachkov, P | |
dc.creator | Browne, F | |
dc.creator | Čeliković, Igor T. | |
dc.creator | de France, G. | |
dc.creator | Doornenbal, P | |
dc.creator | Fang, Y | |
dc.creator | Fukuda, N | |
dc.creator | Giovinazzo, J | |
dc.creator | Goel, N | |
dc.creator | Górska, M | |
dc.creator | Ilieva, S | |
dc.creator | Inabe, N | |
dc.creator | Isobe, T | |
dc.creator | Jungclaus, A | |
dc.creator | Kameda, D | |
dc.creator | Kim, Y. K. | |
dc.creator | Kojouharov, I | |
dc.creator | Kubo, T | |
dc.creator | Kurz, N | |
dc.creator | Kwon, Y. K. | |
dc.creator | Lorusso, G | |
dc.creator | Moschner, K | |
dc.creator | Murai, D | |
dc.creator | Nishizuka, I | |
dc.creator | Patel, Z | |
dc.creator | Rajabali, M. M. | |
dc.creator | Rice, S | |
dc.creator | Schaffner, H | |
dc.creator | Shimizu, Y | |
dc.creator | Sinclair, L | |
dc.creator | Söderström, P.-A. | |
dc.creator | Steiger, K | |
dc.creator | Sumikama, T | |
dc.creator | Suzuki, H | |
dc.creator | Takeda, H | |
dc.creator | Wang, Z | |
dc.creator | Warr, N | |
dc.creator | Watanabe, H | |
dc.creator | Wu, J | |
dc.creator | Xu, Z | |
dc.date.accessioned | 2019-11-12T09:37:18Z | |
dc.date.available | 2019-11-12T09:37:18Z | |
dc.date.issued | 2019 | |
dc.identifier.issn | 0031-9007 | |
dc.identifier.issn | 1079-7114 | |
dc.identifier.uri | https://link.aps.org/doi/10.1103/PhysRevLett.122.222502 | |
dc.identifier.uri | https://vinar.vin.bg.ac.rs/handle/123456789/8339 | |
dc.description.abstract | A record number of Sn100 nuclei was detected and new isotopic species toward the proton dripline were discovered at the RIKEN Nishina Center. Decay spectroscopy was performed with the high-efficiency detector arrays WAS3ABi and EURICA. Both the half-life and the β-decay end point energy of Sn100 were measured more precisely than the literature values. The value and the uncertainty of the resulting strength for the pure 0+→1+ Gamow-Teller decay was improved to BGT=4.4-0.7+0.9. A discrimination between different model calculations was possible for the first time, and the level scheme of In100 is investigated further. © 2019 American Physical Society. | en |
dc.language.iso | en | |
dc.relation | German Research Foundation (DFG) | |
dc.relation | Federal Ministry of Education & Research (BMBF) [05P12WOFNF] | |
dc.relation | Federal Ministry of Education & Research (BMBF) [05P15PKFNA] | |
dc.relation | Hanns-Seidel-Stiftung | |
dc.relation | RIKEN IPA Programme | |
dc.relation | Rare Isotope Science Project - Ministry of Education, Science and Technology, National Research Foundation of Korea-KAKENHI [25247045] | |
dc.relation | Natural Sciences and Engineering Research Council of Canada - FJNSP LIA (French-Japanese International Associated Laboratory for Nuclear Structure Problems) | |
dc.relation | Spanish Ministerio de Economia y Competitividad [FPA2017-84756-C4-2-P] | |
dc.rights | restrictedAccess | |
dc.source | Physical Review Letters | |
dc.subject | Decay spectroscopies | en |
dc.subject | Detector arrays | en |
dc.subject | End points | en |
dc.subject | Half lives | en |
dc.subject | High-efficiency | en |
dc.subject | Isotopic species | en |
dc.subject | Level schemes | en |
dc.subject | Model calculations | en |
dc.title | Improved Value for the Gamow-Teller Strength of the Sn100 Beta Decay | en |
dc.type | article | en |
dc.rights.license | ARR | |
dcterms.abstract | Xу, З; Бланк, Б; де Франце, Г.; Гóрска, М; Кwон, Y. К.; Рајабали, М. М.; Сöдерстрöм, П.-A.; Лубос, Д; Парк, Ј; Фаестерманн, Т; Гернхäусер, Р; Челиковић, Игор Т.; Фукуда, Н; Гиовиназзо, Ј; Гоел, Н; Илиева, С; Инабе, Н; Исобе, Т; Јунгцлаус, A; Камеда, Д; Ким, Y. К.; Којоухаров, И; Кубо, Т; Курз, Н; Лоруссо, Г; Мосцхнер, К; Мураи, Д; Нисхизука, И; Пател, З; Рице, С; Сцхаффнер, Х; Схимизу, Y; Синцлаир, Л; Стеигер, К; Сумикама, Т; Сузуки, Х; Такеда, Х; Wанг, З; Wарр, Н; Wатанабе, Х; Wу, Ј; Баба, Х; Блазхев, A; Боутацхков, П; Броwне, Ф; Доорненбал, П; Фанг, Y; | |
dc.rights.holder | © 2019 American Physical Society | |
dc.citation.volume | 122 | |
dc.citation.issue | 22 | |
dc.citation.spage | 222502 | |
dc.identifier.wos | 000470885800010 | |
dc.identifier.doi | 10.1103/PhysRevLett.122.222502 | |
dc.citation.rank | aM21 | |
dc.identifier.pmid | 31283269 | |
dc.type.version | publishedVersion | |
dc.identifier.scopus | 2-s2.0-85066950864 |
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